Some Properties of Microwave Emission From Flaring Regions

V. R. Maksimov; V.L. Shchepkina; E.A. Chernova

doi:10.11728/cjss2005.05.419

Volume 25 Issue 5

Sep. 2005

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V. R. Maksimov, V.L. Shchepkina, E.A. Chernova. Some Properties of Microwave Emission From Flaring Regions[J]. Chinese Journal of Space Science, 2005, 25(5): 419-423. doi: 10.11728/cjss2005.05.419

Citation:

V. R. Maksimov, V.L. Shchepkina, E.A. Chernova. Some Properties of Microwave Emission From Flaring Regions[J]. Chinese Journal of Space Science, 2005, 25(5): 419-423. doi: 10.11728/cjss2005.05.419

V. R. Maksimov, V.L. Shchepkina, E.A. Chernova. Some Properties of Microwave Emission From Flaring Regions[J]. Chinese Journal of Space Science, 2005, 25(5): 419-423. doi: 10.11728/cjss2005.05.419

Citation:

V. R. Maksimov, V.L. Shchepkina, E.A. Chernova. Some Properties of Microwave Emission From Flaring Regions[J]. Chinese Journal of Space Science, 2005, 25(5): 419-423. doi: 10.11728/cjss2005.05.419

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Some Properties of Microwave Emission From Flaring Regions

doi: 10.11728/cjss2005.05.419

Received Date: 1900-01-01
Rev Recd Date: 1900-01-01
Publish Date: 2005-09-15

Abstract

Abstract

A study is made of the differences in the polarization distribution and other characteristics of microwave emission for several active regionswith high flare productivity. Conclusions are drawn about the magnetic field structure of these regions at coronal heights.
- Microwave emission,
- Solar activity,
- Solar flare prediction